Stellar streams form through the tidal disruption of dwarf galaxies and globular clusters as they accrete onto a larger host galaxy [1]}.
The formation of stellar streams is an expected feature of hierarchical models of galaxy formation where large galaxies grow through mergers of smaller systems [2]}, [3]}.
Due to their formation mechanism, transient nature, and dynamical fragility, stellar streams provide a direct and powerful probe of the gravitational field in galactic halos at both large and small scales [4]}, [5]}, [6]}.
Within our Milky Way in particular, stellar streams have been proposed as sensitive probes of the large- and small-scale distributions of baryonic and dark matter within the Galactic halo [3]}, [8]}, [9]}, [10]}, [11]}.
